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Two years of GRB observations with HETE-2/FREGATE

J L Atteia,C Barraud,John Patrick Lestrade,J P Olive,J P Dezalay,Michel Boer,Kevin C Hurley,J G Jernigan,R George Ricker,Roland Kraft Vanderspek,Geoffrey Crew,John P Doty,Glen Pickslay Monnelly,Jesus Noel Samonte Villasenor,Nathaniel R Butler,Alan M Levine,Nobuyuki Kawai,Atsumasa Yoshida,Taku Sakamoto,T Tamagawa,Kenichi Torii,Masaru Matsuoka,Donald Q Lamb,Timothy Quinn Donaghy,Carlo Alberto Graziani,Graziella Pizzichini,E E Fenimore,Mark Galassi,T Tavenner

ASTRONOMICAL SOCIETY OF THE PACIFIC CONFERENCE SERIES（2004）

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Abstract
We briefly describe the main parameters of the GRBs detected by FREGATE within its field of view during the first two years of its operation (October 2000 - November 2002). This sample includes classical GRBs, X-ray rich GRBs and Short/Hard GRBs. Thanks to the extensive follow-up of HETE-2 GRBs, these observations will allow on the long term to connect the properties of the prompt gamma-ray emission with those of the afterglow for all three types of GRBs.
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Key words
field of view,gamma ray
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